Table 4
Observed source counts, redshift values, and lower limit measurements (uncertain results in parentheses) for different source groups from Paper I, Paper II, Paper III, Goldoni et al. (2024), and the current study (Paper IV).
| Paper (1) | Number of targets (2) | Redshifts (z) (3) | Redshift lower limits (4) | zmed (with limits) (5) | Efficiency (6) |
|---|---|---|---|---|---|
| I | 19(0) | 11 (+1)c | 2(+1)c | 0.21(0.23) | 11/19 |58% |
| II | 25(8) | 14 (+1)c1 | 2 | 0.37(0.38) | 14/25 (33) | 56% (42%) |
| III | 24(17) | 12 (+1) | 2 | 0.39(0.42) | 12/24 (41) | 50% (29%) |
| IV | 29(0) | 12 | 2 | 0.36(0.42) | 12/29 | 41% |
| Combined | 90(25) | 49(+1) | 8 | 0.32/0.36 | 49/90 I 54% |
Notes. The combined results take into account repeated observations (see discussion for details). The columns are as follows: (1) Paper number; (2) Number of observed targets (targets observed with the Lick telescope); (3) Number of measured redshifts; (4) Lower limits on redshift; (5) Median redshift; and (6) Efficiency of redshift detection. Additionally, the combined results of the program, including repeated observations, are presented. The ‘+1’ notation in columns 3 and 4 indicates the inclusion of either additional tentative redshifts or tentative lower limits in the overall count. C & C1: These uncertain results are confirmed in Papers III and Paper IV, respectively.
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